Abstract
This chapter deals with the study of dissipative, locally anisotropic, and spherically symmetric self-gravitating fluids. The analysis is based on a full causal approach, where the dynamical equations are coupled to causal transport equations for the heat flux, shear, and bulk viscosity in the context of the Müller-Israel-Stewart theory by including the thermodynamic viscous/heat coupling coefficients.
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Acknowledgments
I thank my advisors Luis Herrera Cometta and Alicia Di Prisco for their kind support. I also extend my acknowledgements to the organizing committee of the first workshop of the Venezuelan Society of Fluid Mechanics (FLUIDOS2012) for financial support and hospitality during the event.
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Troconis, O. (2014). Dynamics of Relativistic, Dissipative and Anisotropic Self-Gravitating Fluids. In: Sigalotti, L., Klapp, J., Sira, E. (eds) Computational and Experimental Fluid Mechanics with Applications to Physics, Engineering and the Environment. Environmental Science and Engineering(). Springer, Cham. https://doi.org/10.1007/978-3-319-00191-3_39
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DOI: https://doi.org/10.1007/978-3-319-00191-3_39
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